Share Email Print

Proceedings Paper

Improvement of the angular resolution of a thin-foil-nested x-ray telescope
Author(s): Takayuki Hayashi; Takuro Sato; Manabu Ishida; Yoshitomo Maeda; Hideyuki Mori; Ryoko Nakamura; Takayuki Shirata; Kentaro Someya; Yasushi Ogasaka; Kenichi Torii
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

We have been developing a thin-foil-nested X-ray telescope (XRT) for the Japanese X-ray astronomy satellites since ASCA launched in 1993. The thin-foil-nested XRT is advantageous in realizing high throughput with a light weight, whilst its angular resolution is poorer than other mirrors using, for example, a polished thick glass substrate onboard Chandra. We have investigated causes of image degradation of our XRT, and have identified them as figure error and positioning error of the reflectors. Since the latter dominates the entire error budget, we first attempted to improve the positioning error, and adopted the following two methods. First, we substituted an alignment plate for the alignment bar. The alignment plate incorporates the independently movable four alignment bars adopted for ASCA and Suzaku into a single plate. In practice, we allocated a pair of the plate in each slot, and after inserting all the reflectors, we shifted one of the plates radially to tightly hold the reflectors. Second, we have manufactured a partially replicated foil in which reflecting material (Au) is not applied to the axial edges of the foils in order to control the foil position by the edges of the reflectors whose thickness variation is within 2 μm. After these improvements on the positioning error, we moved onto the figure error issue. With X-ray and laser profilometer measurements, we found that the figure error increased in a area closer to the azimuthal edges of the reflector. After considerable struggle for improvement, we finally decided to produce a long reflector and to cut both azimuthal edges. Thanks to these new devices, we have reduced the positioning error from 1.5 arcmin to 0.66. Furthermore, we have successfully produced 40-pairs of reflectors whose figure error is less than 0.8 arcmin. Incorporating these reflectors into a mirror housing, we have measured the XRT performance in the 30 m beamline facility at ISAS/JAXA, and confirmed to achieve an angular resolution of 1.08 arcmin in half-power diameter. The effective area is measured to be 14.0 cm2, which is ~90% of the designed value. Note that this number is significantly enhanced from ~80% in the Suzaku XRT, which is a by-product of the improvement of the angular resolution.

Paper Details

Date Published: 4 September 2009
PDF: 8 pages
Proc. SPIE 7448, Advances in X-Ray/EUV Optics and Components IV, 74480A (4 September 2009); doi: 10.1117/12.826291
Show Author Affiliations
Takayuki Hayashi, Japan Aerospace Exploration Agency (Japan)
Tokyo Metropolitan Univ. (Japan)
Takuro Sato, Japan Aerospace Exploration Agency (Japan)
Tokyo Metropolitan Univ. (Japan)
Manabu Ishida, Japan Aerospace Exploration Agency (Japan)
Tokyo Metropolitan Univ. (Japan)
Yoshitomo Maeda, Japan Aerospace Exploration Agency (Japan)
Hideyuki Mori, Japan Aerospace Exploration Agency (Japan)
Ryoko Nakamura, Japan Aerospace Exploration Agency (Japan)
Takayuki Shirata, Tokyo Metropolitan Univ. (Japan)
Kentaro Someya, Japan Aerospace Exploration Agency (Japan)
Yasushi Ogasaka, Nagoya Univ. (Japan)
Kenichi Torii, Nagoya Univ. (Japan)

Published in SPIE Proceedings Vol. 7448:
Advances in X-Ray/EUV Optics and Components IV
Ali M. Khounsary; Christian Morawe; Shunji Goto, Editor(s)

© SPIE. Terms of Use
Back to Top
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?